Neutrino Quasinormal Modes of a Kerr-Newman-de Sitter Black Hole

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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25 pages, 13 figures

Scientific paper

10.1016/j.nuclphysb.2005.01.043

Using the P\"{o}shl-Teller approximation, we evaluate the neutrino
quasinormal modes (QNMs) of a Kerr-Newman-de Sitter black hole. The result
shows that for a Kerr-Newman-de Sitter black hole, massless neutrino
perturbation of large $\Lambda$, positive $m$ and small value of $n$ will decay
slowly.

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